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FIG. 1.ÈThe 100 kmÈH I correlation with (a) no correction, (b) linear correction, and (c) quadratic correction for zodiacal contamination. The Ðts in the range [0, 200] K km s~1 are shown as solid lines.
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Journal Article
•
DOI
•
Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
[...]
David J. Schlegel
1
,
Douglas P. Finkbeiner
2
,
Marc Davis
2
•
Institutions (2)
Durham University
1
,
University of California, Berkeley
2
28 Oct 1997
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arXiv: Astrophysics